5XMM J123908.5-052256
5XMM-DR15 stacked source · SRCID 3005983010100131
Position:
12h39m08.56s -05d22m56.2s
(189.78569°, -5.38228°)
EP flux
9.10e-15
± 3.7e-15
erg cm-2 s-1
CLASSX
AGN
(0.755)
Detections
8
| SRCID | 3005983010100131 |
|---|---|
| IAUNAME | 5XMM J123908.5-052256 |
| SC_RA | 12h39m08.56s (189.78569°) |
| SC_DEC | -05d22m56.2s (-5.38228°) |
| RADEC_ERR | 1.43 arcsec |
| LII / BII | 297.2524° / 57.3538° |
| N_CONTRIB | 8 (detections) |
| N_OBS | 9 (observations covering the position) |
| MJD_FIRST | 51727.470 (2000-07-02 11:16:21.000 UTC) |
| MJD_LAST | 57585.439 (2016-07-16 10:32:04.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 9.10e-15 ± 3.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.09
± 0.25
0.2-0.5 / 0.5-1.0 keV
HR2
0.31
± 0.19
0.5-1.0 / 1.0-2.0 keV
HR3
-0.59
± 0.20
1.0-2.0 / 2.0-4.5 keV
HR4
0.46
± 0.33
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 1.1)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 1.74
Class probabilities
Class taxonomy
- AGN — active galactic nucleus.
- Bkg_AGN — background AGN.
- Star — Galactic star.
- Gal_XRB — Galactic X-ray binary.
- Extragal_XRB — extragalactic X-ray binary.
- CV — cataclysmic variable.
- Extended — cluster or galaxy.
Optical Monitor (OM)
- OM Source ID
- 3269153
- Match probability
- 0.993
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.325 | 0.380 |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.74e-15 (+4.7e-15 / −2.9e-15) erg cm−2 s−1 |
|---|---|
| NH | 7.70e+19 (+4.1e+20 / −2.0e+19) cm−2 |
| Photon index (Γ) | 2.61 (+2.86 / −2.26) |
| DoF | 67 |
| p-value | 0.552 |
| Quality flag | 0 |
No variability data available for this source.
No contributing observations found.
Sky view (optical)
DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.
Hardness-ratio diagram
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.